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- W2068003834 abstract "THE observation of electromagnetic radiation from the pulsar in the Crab Nebula (NP0532) has been reported over at least 16 decades in energy from the radio band to the high energy γ-ray band1–8. In general, a double pulse structure is evident over this range in energy, although variations in the relative intensities and widths of the two pulses are found. In the optical, X-ray and γ-ray bands the pulsed emission is also seen to spread out into the region between the primary and secondary pulses." @default.
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- W2068003834 date "1973-07-01" @default.
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- W2068003834 title "Arrival Times of 100 to 400 keV Pulses from NP0532" @default.
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- W2068003834 doi "https://doi.org/10.1038/physci244039a0" @default.
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